The MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESI

We present the Multi-Object Spectroscopy of Transient (MOST) Hosts survey. The survey is planned to run throughout the 5 yr of operation of the Dark Energy Spectroscopic Instrument (DESI) and will generate a spectroscopic catalog of the hosts of most transients observed to date, in particular all th...

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Main Authors: Maayane T. Soumagnac, Peter Nugent, Robert A. Knop, Anna Y. Q. Ho, William Hohensee, Autumn Awbrey, Alexis Andersen, Greg Aldering, Matan Ventura, Jessica N. Aguilar, Steven Ahlen, Segev Y. Benzvi, David Brooks, Dillon Brout, Todd Claybaugh, Tamara M. Davis, Kyle Dawson, Axel de la Macorra, Arjun Dey, Biprateep Dey, Peter Doel, Kelly A. Douglass, Jaime E. Forero-Romero, Enrique Gaztañaga, Satya Gontcho A Gontcho, Or Graur, Julien Guy, ChangHoon Hahn, Klaus Honscheid, Cullan Howlett, Alex G. Kim, Theodore Kisner, Anthony Kremin, Andrew Lambert, Martin Landriau, Dustin Lang, Laurent Le Guillou, Marc Manera, Aaron Meisner, Ramon Miquel, John Moustakas, Adam D. Myers, Jundan Nie, Antonella Palmese, David Parkinson, Claire Poppett, Francisco Prada, Fei Qin, Mehdi Rezaie, Graziano Rossi, Eusebio Sanchez, David J. Schlegel, Michael Schubnell, Joseph H. Silber, Gregory Tarlé, Benjamin A. Weaver, Zhimin Zhou
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Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal Supplement Series
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Online Access:https://doi.org/10.3847/1538-4365/ad76ae
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author Maayane T. Soumagnac
Peter Nugent
Robert A. Knop
Anna Y. Q. Ho
William Hohensee
Autumn Awbrey
Alexis Andersen
Greg Aldering
Matan Ventura
Jessica N. Aguilar
Steven Ahlen
Segev Y. Benzvi
David Brooks
Dillon Brout
Todd Claybaugh
Tamara M. Davis
Kyle Dawson
Axel de la Macorra
Arjun Dey
Biprateep Dey
Peter Doel
Kelly A. Douglass
Jaime E. Forero-Romero
Enrique Gaztañaga
Satya Gontcho A Gontcho
Or Graur
Julien Guy
ChangHoon Hahn
Klaus Honscheid
Cullan Howlett
Alex G. Kim
Theodore Kisner
Anthony Kremin
Andrew Lambert
Martin Landriau
Dustin Lang
Laurent Le Guillou
Marc Manera
Aaron Meisner
Ramon Miquel
John Moustakas
Adam D. Myers
Jundan Nie
Antonella Palmese
David Parkinson
Claire Poppett
Francisco Prada
Fei Qin
Mehdi Rezaie
Graziano Rossi
Eusebio Sanchez
David J. Schlegel
Michael Schubnell
Joseph H. Silber
Gregory Tarlé
Benjamin A. Weaver
Zhimin Zhou
author_facet Maayane T. Soumagnac
Peter Nugent
Robert A. Knop
Anna Y. Q. Ho
William Hohensee
Autumn Awbrey
Alexis Andersen
Greg Aldering
Matan Ventura
Jessica N. Aguilar
Steven Ahlen
Segev Y. Benzvi
David Brooks
Dillon Brout
Todd Claybaugh
Tamara M. Davis
Kyle Dawson
Axel de la Macorra
Arjun Dey
Biprateep Dey
Peter Doel
Kelly A. Douglass
Jaime E. Forero-Romero
Enrique Gaztañaga
Satya Gontcho A Gontcho
Or Graur
Julien Guy
ChangHoon Hahn
Klaus Honscheid
Cullan Howlett
Alex G. Kim
Theodore Kisner
Anthony Kremin
Andrew Lambert
Martin Landriau
Dustin Lang
Laurent Le Guillou
Marc Manera
Aaron Meisner
Ramon Miquel
John Moustakas
Adam D. Myers
Jundan Nie
Antonella Palmese
David Parkinson
Claire Poppett
Francisco Prada
Fei Qin
Mehdi Rezaie
Graziano Rossi
Eusebio Sanchez
David J. Schlegel
Michael Schubnell
Joseph H. Silber
Gregory Tarlé
Benjamin A. Weaver
Zhimin Zhou
author_sort Maayane T. Soumagnac
collection DOAJ
description We present the Multi-Object Spectroscopy of Transient (MOST) Hosts survey. The survey is planned to run throughout the 5 yr of operation of the Dark Energy Spectroscopic Instrument (DESI) and will generate a spectroscopic catalog of the hosts of most transients observed to date, in particular all the supernovae observed by most public, untargeted, wide-field, optical surveys (Palomar Transient Factory, PTF/intermediate PTF, Sloan Digital Sky Survey II, Zwicky Transient Facility, DECAT, DESIRT). Science cases for the MOST Hosts survey include Type Ia supernova cosmology, fundamental plane and peculiar velocity measurements, and the understanding of the correlations between transients and their host-galaxy properties. Here we present the first release of the MOST Hosts survey: 21,931 hosts of 20,235 transients. These numbers represent 36% of the final MOST Hosts sample, consisting of 60,212 potential host galaxies of 38,603 transients (a transient can be assigned multiple potential hosts). Of all the transients in the MOST Hosts list, only 26.7% have existing classifications, and so the survey will provide redshifts (and luminosities) for nearly 30,000 transients. A preliminary Hubble diagram and a transient luminosity–duration diagram are shown as examples of future potential uses of the MOST Hosts survey. The survey will also provide a training sample of spectroscopically observed transients for classifiers relying only on photometry, as we enter an era when most newly observed transients will lack spectroscopic classification. The MOST Hosts DESI survey data will be released on a rolling cadence and updated to match the DESI releases. Dates of future releases and updates are available through the https://mosthosts.desi.lbl.gov website.
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spelling doaj-art-a6f6e43e8a48470286b134f6330a81812024-11-12T06:50:38ZengIOP PublishingThe Astrophysical Journal Supplement Series0067-00492024-01-0127522210.3847/1538-4365/ad76aeThe MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESIMaayane T. Soumagnac0https://orcid.org/0000-0001-6753-1488Peter Nugent1https://orcid.org/0000-0002-3389-0586Robert A. Knop2Anna Y. Q. Ho3https://orcid.org/0000-0002-9017-3567William Hohensee4Autumn Awbrey5Alexis Andersen6Greg Aldering7Matan Ventura8Jessica N. Aguilar9https://orcid.org/0000-0003-0822-452XSteven Ahlen10https://orcid.org/0000-0001-6098-7247Segev Y. Benzvi11https://orcid.org/0000-0001-5537-4710David Brooks12https://orcid.org/0000-0002-8458-5047Dillon Brout13https://orcid.org/0000-0001-5201-8374Todd Claybaugh14Tamara M. Davis15https://orcid.org/0000-0002-4213-8783Kyle Dawson16https://orcid.org/0000-0002-0553-3805Axel de la Macorra17https://orcid.org/0000-0002-1769-1640Arjun Dey18https://orcid.org/0000-0002-4928-4003Biprateep Dey19https://orcid.org/0000-0002-5665-7912Peter Doel20Kelly A. Douglass21https://orcid.org/0000-0002-9540-546XJaime E. Forero-Romero22https://orcid.org/0000-0002-2890-3725Enrique Gaztañaga23https://orcid.org/0000-0001-9632-0815Satya Gontcho A Gontcho24Or Graur25Julien Guy26https://orcid.org/0000-0001-9822-6793ChangHoon Hahn27https://orcid.org/0000-0003-1197-0902Klaus Honscheid28Cullan Howlett29https://orcid.org/0000-0002-1081-9410Alex G. Kim30https://orcid.org/0000-0001-6315-8743Theodore Kisner31https://orcid.org/0000-0003-3510-7134Anthony Kremin32https://orcid.org/0000-0001-6356-7424Andrew Lambert33Martin Landriau34https://orcid.org/0000-0003-1838-8528Dustin Lang35Laurent Le Guillou36https://orcid.org/0000-0001-7178-8868Marc Manera37https://orcid.org/0000-0003-4962-8934Aaron Meisner38https://orcid.org/0000-0002-1125-7384Ramon Miquel39https://orcid.org/0000-0002-6610-4836John Moustakas40https://orcid.org/0000-0002-2733-4559Adam D. Myers41Jundan Nie42https://orcid.org/0000-0001-6590-8122Antonella Palmese43https://orcid.org/0000-0002-6011-0530David Parkinson44https://orcid.org/0000-0002-7464-2351Claire Poppett45https://orcid.org/0000-0003-0512-5489Francisco Prada46https://orcid.org/0000-0001-7145-8674Fei Qin47https://orcid.org/0000-0001-7950-7864Mehdi Rezaie48https://orcid.org/0000-0001-5589-7116Graziano Rossi49Eusebio Sanchez50https://orcid.org/0000-0002-9646-8198David J. Schlegel51https://orcid.org/0000-0002-5042-5088Michael Schubnell52Joseph H. Silber53https://orcid.org/0000-0002-3461-0320Gregory Tarlé54https://orcid.org/0000-0003-1704-0781Benjamin A. Weaver55Zhimin Zhou56https://orcid.org/0000-0002-4135-0977Department of Physics, Bar-Ilan University , Israel ; mtsoumagnac@lbl.gov; Lawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA; Department of Astronomy, University of California, Berkeley , Berkeley, CA 94720-3411, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Astronomy, Cornell University , Ithaca, NY 14853, USADepartment of Astronomy, University of California, Berkeley , Berkeley, CA 94720-3411, USADepartment of Astronomy, University of California, Berkeley , Berkeley, CA 94720-3411, USADepartment of Astronomy, University of California, Berkeley , Berkeley, CA 94720-3411, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Physics, Bar-Ilan University , Israel ; mtsoumagnac@lbl.govLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Physics, Boston University , Boston, MA 02115, USADepartment of Physics & Astronomy, University of Rochester , Rochester, 206 Bausch and Lomb Hall, P.O. Box 270171, Rochester, NY 14627-0171, USADepartment of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UKDepartment of Physics, Boston University , Boston, MA 02115, USA; Department of Astronomy, Boston University , Boston, MA 02115, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USASchool of Mathematics and Physics, The University of Queensland , St Lucia, QLD 4101, AustraliaDepartment of Physics and Astronomy, The University of Utah , 115 South 1400 East, Salt Lake City, UT 84112, USAInstituto de Física, Universidad Nacional Autónoma de Mexico , Cd. de Mexico C.P. 04510, MexicoNSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USADepartment of Physics & Astronomy and Pittsburgh Particle Physics, Astrophysics, and Cosmology Center (PITT PACC), University of Pittsburgh , 3941 O’Hara Street, Pittsburgh, PA 15260, USADepartment of Physics & Astronomy, University College London , Gower Street, London, WC1E 6BT, UKDepartment of Physics & Astronomy, University of Rochester , Rochester, 206 Bausch and Lomb Hall, P.O. Box 270171, Rochester, NY 14627-0171, USADepartamento de Física, Universidad de los Andes , Cra. 1 No. 18A-10, Edificio Ip, CP 111711, Bogotá, Colombia; Observatorio Astronómico, Universidad de los Andes , Cra. 1 No. 18A-10, Edificio H, CP 111711 Bogotá, ColombiaInstitut d’Estudis Espacials de Catalunya (IEEC) , 08034 Barcelona, Spain; Institute of Cosmology & Gravitation, University of Portsmouth , Dennis Sciama Building, Portsmouth, PO1 3FX, UK; Institute of Space Sciences , ICE-CSIC, Campus UAB, Carrer de Can Magrans s/n, 08913 Bellaterra, Barcelona, SpainLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA; Department of Physics & Astronomy, University of Rochester , Rochester, NY 14627, USAInstitute of Cosmology and Gravitation, University of Portsmouth , Portsmouth, PO1 3FX, UK; Department of Astrophysics, American Museum of Natural History, Central Park West and 79th Street , New York, NY 10024, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Astrophysical Sciences, Princeton University , Princeton NJ 08544, USACenter for Cosmology and AstroParticle Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USA; Department of Physics, The Ohio State University , 191 West Woodruff Avenue, Columbus, OH 43210, USA; The Ohio State University , Columbus, OH 43210, USASchool of Mathematics and Physics, The University of Queensland , St Lucia, QLD 4101, AustraliaLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADunlap Institute, University of Toronto , Toronto, ON M5S 3H4, Canada; Department of Astronomy & Astrophysics, University of Toronto , Toronto, ON M5S 3H4, Canada; Perimeter Institute for Theoretical Physics , Waterloo, ON N2L 2Y5, CanadaSorbonne Université , CNRS/IN2P3, Laboratoire de Physique Nucléaire et de Hautes Energies (LPNHE), FR-75005 Paris, FranceDepartament de Física, Serra Húnter, Universitat Autònoma de Barcelona , 08193 Bellaterra (Barcelona), Spain; Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, 08193 Bellaterra Barcelona, SpainNSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USAInstitut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology , Campus UAB, 08193 Bellaterra Barcelona, Spain; Institució Catalana de Recerca i Estudis Avançats , Passeig de Lluís Companys, 23, 08010 Barcelona, SpainDepartment of Physics and Astronomy, Siena College , 515 Loudon Road, Loudonville, NY 12211, USADepartment of Physics & Astronomy, University of Wyoming , 1000 E. University, Dept. 3905, Laramie, WY 82071, USANational Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing, 100012, People's Republic of ChinaLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA; McWilliams Center for Cosmology, Department of Physics, Carnegie Mellon University , Pittsburgh, PA 15213, USA; Department of Physics, University of California, Berkeley , Berkeley, CA, 94720-3411, USAKorea Astronomy and Space Science Institute , 776, Daedeokdae-ro, Yuseong-gu, Daejeon 34055, Republic of KoreaLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USA; Space Sciences Laboratory, University of California , Berkeley, 7 Gauss Way, Berkeley, CA 94720, USA; University of California , Berkeley, 110 Sproul Hall #5800, Berkeley, CA 94720, USAInstituto de Astrofísica de Andalucía (CSIC) , Glorieta de la Astronomía, s/n, E-18008 Granada, SpainSchool of Physics, Korea Institute for Advanced Study , Hoegiro 85, Dongdaemun-gu, Seoul 02455, Republic of KoreaDepartment of Physics, Kansas State University , 116 Cardwell Hall, Manhattan, KS 66506, USADepartment of Physics and Astronomy, Sejong University , Seoul, 143-747, Republic of KoreaCIEMAT , Avenida Complutense 40, E-28040 Madrid, SpainLawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USADepartment of Physics, University of Michigan , Ann Arbor, MI 48109, USA; University of Michigan , Ann Arbor, MI 48109, USALawrence Berkeley National Laboratory , 1 Cyclotron Road, Berkeley, CA 94720, USAUniversity of Michigan , Ann Arbor, MI 48109, USANSF’s NOIRLab , 950 N. Cherry Avenue, Tucson, AZ 85719, USANational Astronomical Observatories, Chinese Academy of Sciences , A20 Datun Road, Chaoyang District, Beijing, 100012, People's Republic of ChinaWe present the Multi-Object Spectroscopy of Transient (MOST) Hosts survey. The survey is planned to run throughout the 5 yr of operation of the Dark Energy Spectroscopic Instrument (DESI) and will generate a spectroscopic catalog of the hosts of most transients observed to date, in particular all the supernovae observed by most public, untargeted, wide-field, optical surveys (Palomar Transient Factory, PTF/intermediate PTF, Sloan Digital Sky Survey II, Zwicky Transient Facility, DECAT, DESIRT). Science cases for the MOST Hosts survey include Type Ia supernova cosmology, fundamental plane and peculiar velocity measurements, and the understanding of the correlations between transients and their host-galaxy properties. Here we present the first release of the MOST Hosts survey: 21,931 hosts of 20,235 transients. These numbers represent 36% of the final MOST Hosts sample, consisting of 60,212 potential host galaxies of 38,603 transients (a transient can be assigned multiple potential hosts). Of all the transients in the MOST Hosts list, only 26.7% have existing classifications, and so the survey will provide redshifts (and luminosities) for nearly 30,000 transients. A preliminary Hubble diagram and a transient luminosity–duration diagram are shown as examples of future potential uses of the MOST Hosts survey. The survey will also provide a training sample of spectroscopically observed transients for classifiers relying only on photometry, as we enter an era when most newly observed transients will lack spectroscopic classification. The MOST Hosts DESI survey data will be released on a rolling cadence and updated to match the DESI releases. Dates of future releases and updates are available through the https://mosthosts.desi.lbl.gov website.https://doi.org/10.3847/1538-4365/ad76aeTransient sourcesSurveysSky surveysRedshift surveysGalaxy spectroscopy
spellingShingle Maayane T. Soumagnac
Peter Nugent
Robert A. Knop
Anna Y. Q. Ho
William Hohensee
Autumn Awbrey
Alexis Andersen
Greg Aldering
Matan Ventura
Jessica N. Aguilar
Steven Ahlen
Segev Y. Benzvi
David Brooks
Dillon Brout
Todd Claybaugh
Tamara M. Davis
Kyle Dawson
Axel de la Macorra
Arjun Dey
Biprateep Dey
Peter Doel
Kelly A. Douglass
Jaime E. Forero-Romero
Enrique Gaztañaga
Satya Gontcho A Gontcho
Or Graur
Julien Guy
ChangHoon Hahn
Klaus Honscheid
Cullan Howlett
Alex G. Kim
Theodore Kisner
Anthony Kremin
Andrew Lambert
Martin Landriau
Dustin Lang
Laurent Le Guillou
Marc Manera
Aaron Meisner
Ramon Miquel
John Moustakas
Adam D. Myers
Jundan Nie
Antonella Palmese
David Parkinson
Claire Poppett
Francisco Prada
Fei Qin
Mehdi Rezaie
Graziano Rossi
Eusebio Sanchez
David J. Schlegel
Michael Schubnell
Joseph H. Silber
Gregory Tarlé
Benjamin A. Weaver
Zhimin Zhou
The MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESI
The Astrophysical Journal Supplement Series
Transient sources
Surveys
Sky surveys
Redshift surveys
Galaxy spectroscopy
title The MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESI
title_full The MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESI
title_fullStr The MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESI
title_full_unstemmed The MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESI
title_short The MOST Hosts Survey: Spectroscopic Observation of the Host Galaxies of ∼40,000 Transients Using DESI
title_sort most hosts survey spectroscopic observation of the host galaxies of ∼40 000 transients using desi
topic Transient sources
Surveys
Sky surveys
Redshift surveys
Galaxy spectroscopy
url https://doi.org/10.3847/1538-4365/ad76ae
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